Photometry of a group of stars in the direction of NGC 1746/1750/1758

Document Type

Article

Publication Date

9-1-2010

Abstract

UBV broadband photometry is reported for 19 stars in the direction of the Galactic (open) star clusters NGC 1746/1750/1758. Nine of these stars possess proper motions that point to the existence of a group centered at α = 05h04m and δ = +23°43.5′. One known variable star, V1153 Tau, is recovered, and an emissionline star, HD 32318, is shown to be a variable star. RT Tau is reconfirmed to be constant in light. © 2010. The Astronomical Society of the Pacific. All rights reserved.

Publication Source (Journal or Book title)

Publications of the Astronomical Society of the Pacific

First Page

1008

Last Page

1014

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